Summary table |
Variable |
Value |
Source |
GRB_name_Fermi |
GRB100223110 |
|
T0 |
2:38:09.242 UTC |
Fermi_GBM |
ra |
104.5000° |
Fermi_GBM |
decl |
3.7000° |
Fermi_GBM |
pos_error |
5.61e+00° |
Fermi_GBM |
T90 |
0.256 s |
Fermi_GBM |
T90_error |
0.091 s |
Fermi_GBM |
T90_start |
2:38:09.242 UTC |
Fermi_GBM |
fluence |
1.50e-06 erg/cm² |
Fermi_GBM |
fluence_error |
1.13e-08 erg/cm² |
Fermi_GBM |
T100 |
0.256 s |
|
GBM_located |
True |
|
mjd |
55250.109829189816 |
Fermi_GBM |
Fermi GBM table |
GRB_name_Fermi |
GRB100223110 |
trigger_name |
bn100223110 |
ra |
104.5000° |
decl |
3.7000° |
pos_error |
5.61e+00° |
datum |
2010-02-23 |
t_trigger |
2:38:09.306 UTC |
T90 |
0.256 s |
T90_error |
0.091 s |
T90_start |
2:38:09.242 UTC |
fluence |
1.50e-06 erg/cm² |
fluence_error |
1.13e-08 erg/cm² |
flux_1024 |
3.09e+00 erg/cm²/s |
flux_1024_error |
2.01e-01 erg/cm²/s |
flux_1024_time |
-1.92e-01 erg/cm²/s |
flux_64 |
1.86e+01 erg/cm²/s |
flux_64_error |
1.90e+00 erg/cm²/s |
GCN 10448 table |
GRB_name |
GRB100223A |
GCN_number |
10448 |
Detection_method |
Fermi GBM Det |
t_trigger |
2:38:09.310 UTC |
ra |
104.1000° |
decl |
2.8000° |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 10448
SUBJECT: GRB 100223A: Fermi GBM detection
DATE: 10/02/24 03:27:41 GMT
FROM: Sylvain Guiriec at UAH
Colleen Wilson-Hodge (NASA) and Sylvain Guiriec (UAH)
report on behalf of the Fermi GBM Team:
"At 02:38:09.31 UT on 23 February 2010, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 100223A (trigger 288585491 / 100223110).
The on-ground calculated location, using the GBM trigger
data, is RA = 104.1, DEC = +2.8 (J2000 degrees,
equivalent to 6 h 56 m, 2 d 48 '), with an uncertainty
of 3.6 degrees (radius, 1-sigma containment,
statistical only; there is additionally a systematic
error which is currently estimated to be 2 to 3 degrees).
The angle from the Fermi LAT boresight is 76 degrees.
GBM triggered on a soft peak lasting about 0.05 s followed few ms later by
a longer and harder one. The T90 duration is about 0.206 s (50-300 keV).
The time-averaged spectrum from T0-0.01 s to T0+0.22 s is
adequately fit by a power law function with an exponential
high energy cutoff. The power law index is -0.31 +/- 0.08 and
the cutoff energy, parameterized as Epeak, is 1143 +/- 109 keV
(Castor C-stat 570.83 for 605 d.o.f.).
The event fluence (10-1000 keV) in this time interval is
(1.42 +/- 0.04)E-06 erg/cm^2. The 1-sec peak photon flux measured
starting from T0-0.01 s in the 10-1000 keV band
is 12.5 +/- 0.4 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
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